Photoheliograph
Full-disk solar imaging in white light for sunspot and facular studies.
About the project
A scientific platform for studying solar activity: an interactive three-dimensional map and observational series spanning more than 100 years.
The project is based on observations from the Kislovodsk Mountain Astronomical Station of GAO RAS. We combine them with archival data from other observatories, assembling long series for studying changes in solar activity.
The project is still in development, and we welcome your feedback at iberalex@ya.ru, ivnbrzn@gmail.com
Chromospheric Hα Telescope
Chromospheric observations in hydrogen Hα to trace filaments, prominences and plages.
Small Lyot Coronagraph
Spectral measurements in the Fe X and Fe XIV lines around the solar limb, probing coronal plasma structures.
Ca II K Tower Spectroheliograph
Spectroheliograms in the ionized calcium Ca II K line, sensitive to the chromospheric network and plages.
Radio telescope RT-2
Radio emission measurements at 3.2 cm, probing active regions and solar radio bursts.
Radio telescope RT-3
Radio emission measurements at 4.9 cm, probing active regions and solar radio bursts.
STOP magnetograph
Full-disk magnetic field measurements in the Fe I 630.25 nm line, mapping the photospheric magnetic field.
SPOT Ca II K
Full-disk spectroheliograms in the Ca II K line, enabling high-cadence monitoring of chromospheric activity and eruptions.
SPOT Hα
Full-disk spectroheliograms in the Hα line, enabling high-cadence monitoring of chromospheric activity and eruptions.
SAM Magnetometer
Geomagnetic field measurements, tracking temporal variations of the Earth's magnetic field.